Numerical modelling of spectral line asymmetries in photospheric structures. II. Plage regions.
A numerical code has been developed for modelling the asymmetries in three spectral lines (K I 7699, Fe I 5576 and Fe I 5635A) formed at different photospheric heights and observed in plage regions near the solar disk center. The aim of this work was to reproduce the absolute line bisectors obtained from low resolution observations. The mere
Marquez, I. et al.
Fecha de publicación:
2
1996